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researcher

S. Borisov

13 papers hereh-index 437 citations14 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author6
  • last author5

Across the 13 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM8
  • astro-ph.GA3
  • astro-ph.SR2
same name
  • S. Borisov — 11 papers, h 21
  • S. Borisov — 7 papers, h 5
  • S. Borisov — 4 papers, h 2
  • S. Borisov — 2 papers, h 59
  • S. Borisov — 1 paper, h 9

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20212026
most citedLithium depletion and angular momentum transport in F-type and G-type stars in Galactic open clusters

30 citations · 58 across the 13 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2024

A closer look at the extended edge-on low-surface brightness galaxies

Anna S. Saburova, Damir Gasymov, Evgenii V. Rubtsov +13

To understand the origin of extended disks of low-surface brightness (LSB) galaxies, we studied in detail 4 such systems with large disks seen edge-on. Two of them are edge-on gian…

astro-ph.GA2023

\HI{} 21cm observations and dynamical modelling of the thinnest galaxy: FGC 2366

K. Aditya, Arunima Banerjee, Peter Kamphuis +3

Superthin galaxies are bulgeless low surface brightness galaxies with unusually high major-to-minor axes ratio of the stellar disc, i.e.,10<a/b<20. We present Giant Metrewave Rad…

astro-ph.GA2021★ 5 cited

HI 21 cm observation and mass models of the extremely thin galaxy FGC 1440

K. Aditya, Peter Kamphuis, Arunima Banerjee +4

We present observations and models of the kinematics and distribution of neutral hydrogen (HI) in the superthin galaxy FGC 1440 with an optical axial ratio a/b=20.4. Using the…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.